Paper Citation Record · LEDGER

Massive star cluster origin for the galactic cosmic ray population at very-high energies

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2211.11625.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2211.11625 v2

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:26:47.671536Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-03T02:57:35.353965Z

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1a51f9a6-13a3-4ad9-aaaf-5a559b461793 · inbound

SAETASS: Solver for Astroparticle Equation of Transport Analysis in Spherical Symmetry cites this paper.

SAETASS: Solver for Astroparticle Equation of Transport Analysis in Spherical Symmetry Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-11T12:26:12.378987Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 6ea266d1-529d-4110-923e-6f518bfac3d6 · inbound

Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays cites this paper.

Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 22

Resolution: verified exact; arxiv_id, observed 2026-07-01T20:06:11.956805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation c801793c-d0f8-4b4c-bb6e-f71b9cc20df5 · inbound

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays cites this paper.

Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-07-03T02:57:35.355515Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 7fd7be19-bcac-4a7e-98f1-4941b011bcb0 · inbound

Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region cites this paper.

Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T02:23:17.644495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f07913a1-616b-4a63-920a-b97daaed1447 · inbound

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding cites this paper.

CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 145

Resolution: unresolved; no resolver link, observed 2026-08-02T02:26:47.671536Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation da82a444-21fa-4ee9-9b6d-e4941e5ba3bc · inbound

A cosmic-ray loaded nascent outflow driven by a massive star cluster cites this paper.

A cosmic-ray loaded nascent outflow driven by a massive star cluster Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T22:21:55.676365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6bf8a573-06be-4ef5-b8c7-ee604d2e258a · inbound

Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 cites this paper.

Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 Massive star cluster origin for the galactic cosmic ray population at very-high energies

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T21:55:38.188728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.